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Glossary term: A型星

Description: A型星是指光谱类型为“A“的恒星。天文学家通过A型星光谱中存在的非常强的氢吸收线来识别它们。它们的典型(有效)温度在7400 K到10,000 K之间。与其他恒星相比,除非受到星际或大气层红化的影响,否则它们在人眼中呈现白色或蓝白色。天狼星是夜空中最亮的恒星,而织女星是所有其他恒星在视星等尺度上衡量其他星亮度的标准星,它们都是A型星。

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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

Related Diagrams

A 型恒星的光谱

Caption: A 型恒星 BD-11 1212 的光谱。波长在 400 纳米到 700 纳米之间的光谱线的颜色与人眼看到的该波长光线的颜色大致对应。在 400 纳米以下和 700 纳米以上,人眼几乎看不到光,光谱线分别被染成蓝色和红色。 黑线表示恒星大气中不同元素的原子和离子造成的光谱吸收线。这些原子和离子会吸收特定波长的光,从而在光谱中形成尖锐的暗线。这些线条的强度取决于恒星大气层的温度。如果两颗恒星的大气层温度不同,那么由相同元素混合而成的两颗恒星的光谱中可能会出现截然不同的光谱线。来自氢原子的光谱线在 A 型恒星的光谱中占主导地位,并且在这种光谱类型中最强。
Credit: IAU OAE/SDSS/Niall Deacon

License: CC-BY-4.0 Creative Commons 署名 4.0 国际 (CC BY 4.0) icons